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molecules:ism:cncn [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:cncn [2019/10/22 17:11] (current) – mueller | ||
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M. Agúndez, N. Marcelino, and J. Cernicharo, | M. Agúndez, N. Marcelino, and J. Cernicharo, | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://dx.doi.org/10.1051/0004-6361/201526317|Discovery of Interstellar Isocyanogen (CNCN): Further Evidence that Dicyanopolyynes Are Abundant in Space]]**\\ | + | **[[https:// |
// | // | ||
The IRAM 30 m telescope was used to detect three transitions out of four transitions with //J// = 8 – 7 near 82.8 GHz to //J// = 11 – 10 near 113.8 GHz toward the the young stellar object IRAS 18148–0440 in the L483 dense core. The signal-to-noise (S/N) ratios were reasonable to good for the first three transitions, | The IRAM 30 m telescope was used to detect three transitions out of four transitions with //J// = 8 – 7 near 82.8 GHz to //J// = 11 – 10 near 113.8 GHz toward the the young stellar object IRAS 18148–0440 in the L483 dense core. The signal-to-noise (S/N) ratios were reasonable to good for the first three transitions, | ||
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Contributor(s): | Contributor(s): | ||
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